MRI and outflows: Angular momentum transport in protoplanetary disks

Raquel Salmeron

doi:10.1007/978-3-642-00576-3_92

MRI and outflows: Angular momentum transport in protoplanetary disks

Raquel Salmeron^*

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Chapter › peer-review

Abstract

Angular momentum in protostellar disks can be transported radially by MHD turbulence induced by the magnetorotational instability (MRI); or vertically, via magnetocentrifugal outflows. We have studied these processes under realistic fluid conditions and explored the possibility that they operate at the same radial location. The results suggest that they may be unlikely to coexist in real disks.

Original language	English
Title of host publication	Astrophysics and Space Science Proceedings
Publisher	Springer Science and Business Media B.V.
Pages	611-613
Number of pages	3
Edition	9783642005756
ISBN (Electronic)	9783642005763
ISBN (Print)	9780387727677, 9780387876207, 9781402055720, 9781402069321, 9781402088674, 9781402091896, 9781441981608, 9781441983688, 9783540758259, 9783642005756, 9783642033230, 9783642103216, 9783642103513, 9783642113406, 9783642172502, 9789048133994, 9789048134984
DOIs	https://doi.org/10.1007/978-3-642-00576-3_92
Publication status	Published - 2009

Publication series

Name	Astrophysics and Space Science Proceedings
Number	9783642005756
Volume	0
ISSN (Print)	1570-6591
ISSN (Electronic)	1570-6605

Access to Document

10.1007/978-3-642-00576-3_92

Cite this

@inbook{6c0b8cfde4d54ac49e75626768e87be4,

title = "MRI and outflows: Angular momentum transport in protoplanetary disks",

abstract = "Angular momentum in protostellar disks can be transported radially by MHD turbulence induced by the magnetorotational instability (MRI); or vertically, via magnetocentrifugal outflows. We have studied these processes under realistic fluid conditions and explored the possibility that they operate at the same radial location. The results suggest that they may be unlikely to coexist in real disks.",

author = "Raquel Salmeron",

note = "Publisher Copyright: {\textcopyright} Springer-Verlag Berlin Heidelberg 2009.",

year = "2009",

doi = "10.1007/978-3-642-00576-3_92",

language = "English",

isbn = "9780387727677",

series = "Astrophysics and Space Science Proceedings",

publisher = "Springer Science and Business Media B.V.",

number = "9783642005756",

pages = "611--613",

booktitle = "Astrophysics and Space Science Proceedings",

address = "Germany",

edition = "9783642005756",

}

MRI and outflows: Angular momentum transport in protoplanetary disks. / Salmeron, Raquel.
Astrophysics and Space Science Proceedings. 9783642005756. ed. Springer Science and Business Media B.V., 2009. p. 611-613 (Astrophysics and Space Science Proceedings; Vol. 0, No. 9783642005756).

Research output: Chapter in Book/Report/Conference proceeding › Chapter › peer-review

TY - CHAP

T1 - MRI and outflows

T2 - Angular momentum transport in protoplanetary disks

AU - Salmeron, Raquel

N1 - Publisher Copyright: © Springer-Verlag Berlin Heidelberg 2009.

PY - 2009

Y1 - 2009

N2 - Angular momentum in protostellar disks can be transported radially by MHD turbulence induced by the magnetorotational instability (MRI); or vertically, via magnetocentrifugal outflows. We have studied these processes under realistic fluid conditions and explored the possibility that they operate at the same radial location. The results suggest that they may be unlikely to coexist in real disks.

AB - Angular momentum in protostellar disks can be transported radially by MHD turbulence induced by the magnetorotational instability (MRI); or vertically, via magnetocentrifugal outflows. We have studied these processes under realistic fluid conditions and explored the possibility that they operate at the same radial location. The results suggest that they may be unlikely to coexist in real disks.

UR - http://www.scopus.com/inward/record.url?scp=85032441876&partnerID=8YFLogxK

U2 - 10.1007/978-3-642-00576-3_92

DO - 10.1007/978-3-642-00576-3_92

M3 - Chapter

SN - 9780387727677

SN - 9780387876207

SN - 9781402055720

SN - 9781402069321

SN - 9781402088674

SN - 9781402091896

SN - 9781441981608

SN - 9781441983688

SN - 9783540758259

SN - 9783642005756

SN - 9783642033230

SN - 9783642103216

SN - 9783642103513

SN - 9783642113406

SN - 9783642172502

SN - 9789048133994

SN - 9789048134984

T3 - Astrophysics and Space Science Proceedings

SP - 611

EP - 613

BT - Astrophysics and Space Science Proceedings

PB - Springer Science and Business Media B.V.

ER -

MRI and outflows: Angular momentum transport in protoplanetary disks

Abstract

Publication series

Access to Document

Other files and links

Fingerprint

Cite this